"There are infinite worlds both like and unlike this world of ours ... we must believe that in all worlds there are living creatures and plants and other things we see in this world".... Epicurus (341-270 BC).

Since the times of the ancient greeks, and likely since we became sentient human beings, there has been the longing, or at least the curiosity, to know if we are alone in the universe, or if there are other beings on other
planets. We may find out in our lifetimes.

Planet Transit
About 10 years ago, several techniques were developed to determine if stars, other than our star -- the sun -- had planets. The first method, as you can see by the picture on the left, what we do is to look at a star and see if the light dims and then brightens as we look at it for a long enough time. This would indicate a planet (or planets) in orbit around the star. This method is called the "Transit" method.

The second, more sophisticated method is where we look at the light change in the star, and if we see red light then blue light, this also means that something is orbiting. This "Radial Method" relies on the Doppler effect (or shift). The Doppler effect is that objects moving fast towards us show more as red light and objects moving away from us show more blue light.

The third method is to look for an odd-shaped star that has a ring around it that could be a system of comets and asteroids, much like our solar system.

Since we began looking, we have found over 340 such planets. We call these -- exo-planets or extrasolar planets (Scientists can't agree). We have also found a handful of exo-solar systems -- where a star has multiple planets orbiting. In the 10 years, the space agencies have enlisted the help of amateur astronomers world-wide to track stars and report findings. People take images after images and studied for signs of apparent change in brightness of a star.

Another milestone. When the
Hubble Space Telescope was launched in 1990, we had not yet discovered a single exo-planet. Now - 20 years later, Hubble is being used to determine the atmospheres of exo-planetts.

This may appear somewhat tedious. But then you find something like
Formalhaut! Most exo-planets have been found using the Radial method, so far.

However, with these techniques, we are likely to mainly find the most massive of planets, as planets are much smaller than the stars they orbit. For example, if you were to see the transit of our largest planet, Jupiter, across our star, the Sun, it would only block 1% of sunlight. So almost all of the exo-planets we have found are huge. Most of these orbit close in to their stars and must be incredibly hot, so in the community of scientists involved in this hunt, they are called "roasters".

Venus Transit
This image shows what Venus looks like when it transits our sun.

exo-planet vs Venus Transit
So far, there has been only a few exceptions to this: ESA's CoRoT spacecraft has recently discovered a star with a planet only twice that of Earth. The image on the left shows the star (right side), and a comparison to a Venus/Mercury transit (left side). So things are getting interesting! Click here to see a little movie describing the CoRoT mission.

Previously, it discovered a planet only 5 times the size of Earth. These planets orbit a star named Gliese. Gliese, we now know has at least 3 planets and this last find maybe the first discovery of a habitable planet.

What is our criteria for determining if a planet is habitable? The image below depicts our current criteria:

Our Solar System

So, we are looking for planets as follows (M= Mass e= Earth, H= Hydrogen and He= Helium):

Habitables Area

NASA has just launched a
new space telescope that, among other work, will relieve this tedious task. Kepler, due to launch in early March 2009, will focus on an area of the sky in the Orion constellation, and can simultaneously watch 100,000 stars! This is a profound mission. By observing more than 100,000 stars, Kepler will make statistically significant measurements of the frequency with which terrestrial planets orbit in the habitable zones of stars in the galaxy. If such planets are common, Kepler will detect hundreds of them. If Kepler detects none, then Earth-like planets are very rare, and we may be alone in the galaxy.

The next two images show the size and structure of the telescope (compare the telescope to the size of the technician working on it:

Kepler Side 1 Kepler Side 2

The following images show the area of the sky where Kepler will observe. This area was selected as it has a lot of stars similar in size to ours, plus it is an area of space where NASA's Deep Space Network can track it:

The Red Square shows where Kepler will Observe

Within the red frame of the picture above, This is where Kepler will work:

Kepler's Field of View

The next image shows an artist's rendition of this location in our galaxy (The Milky Way):

Relative area in our Galaxy

Finally, Kepler will hopefully answer our age old question: